Currently three isolated radio pulsars and one binary radio pulsar with no evidence of any previous recycling are known in 97 surveyed Galactic globular clusters (GCs). As pointed out by Lyne et al., the presence of these pulsars cannot be explained by core-collapse supernovae, as commonly assumed for their counterparts in the Galactic disk. We apply a Bayesian analysis to the results from surveys for radio pulsars in GCs and find the number of potentially observable non-recycled radio pulsars present in all clusters to be more » - 0.6. In this case, the potentially observable population of such young pulsars is 447{sup +1420}{sub -399} (the error bars give a 95% confidence interval) and their birthrate is 0.012{sup +0.037}{sub -0.010} puls...
This version implements a number of small corrections to the text which were recently submitted as a...
We report the discovery of two highly dispersed pulsars in the direction of the Galactic Centre made...
We present the discovery and follow-up observations of 142 pulsars found in the Parkes 20-cm multibe...
We explore the enigmatic population of long-period, apparently non-recycled pulsars in globular clus...
Pulsars are interesting astronomical objects in their own right but, they are also great instruments...
Most of the ~600 known pulsars are single and located in the disk of our Galaxy. There is circumsta...
International audienceThe population of young, non-recycled pulsars with spin-down energies |$\dot{E...
Globular clusters are highly efficient radio pulsar factories. These pulsars can be used as precisio...
We investigate the pulsar birthrate from a sample of 815 nonrecycled pulsars detected by the Parkes ...
Although high-sensitivity surveys have revealed a number of highly dispersed pulsars in the inner Ga...
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
The Parkes Multibeam Pulsar Survey has unlocked vast areas of the Galactic plane, which were previou...
We present a Chandra X-ray survey of the disrupted recycled pulsars (DRPs), isolated radio pulsars w...
Millisecond pulsars are conventionally assumed to be spun up through the action of binary companion...
The most massive globular cluster in our Galaxy, Omega Centauri, is aninteresting target for pulsar ...
This version implements a number of small corrections to the text which were recently submitted as a...
We report the discovery of two highly dispersed pulsars in the direction of the Galactic Centre made...
We present the discovery and follow-up observations of 142 pulsars found in the Parkes 20-cm multibe...
We explore the enigmatic population of long-period, apparently non-recycled pulsars in globular clus...
Pulsars are interesting astronomical objects in their own right but, they are also great instruments...
Most of the ~600 known pulsars are single and located in the disk of our Galaxy. There is circumsta...
International audienceThe population of young, non-recycled pulsars with spin-down energies |$\dot{E...
Globular clusters are highly efficient radio pulsar factories. These pulsars can be used as precisio...
We investigate the pulsar birthrate from a sample of 815 nonrecycled pulsars detected by the Parkes ...
Although high-sensitivity surveys have revealed a number of highly dispersed pulsars in the inner Ga...
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
The Parkes Multibeam Pulsar Survey has unlocked vast areas of the Galactic plane, which were previou...
We present a Chandra X-ray survey of the disrupted recycled pulsars (DRPs), isolated radio pulsars w...
Millisecond pulsars are conventionally assumed to be spun up through the action of binary companion...
The most massive globular cluster in our Galaxy, Omega Centauri, is aninteresting target for pulsar ...
This version implements a number of small corrections to the text which were recently submitted as a...
We report the discovery of two highly dispersed pulsars in the direction of the Galactic Centre made...
We present the discovery and follow-up observations of 142 pulsars found in the Parkes 20-cm multibe...